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<ri:Resource created="2012-02-02T14:40:06Z" status="active" updated="2026-07-02T11:57:44Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>VLBI and bright Fermi/LAT sources</title><shortName>J/ApJ/707/L56</shortName><identifier>ivo://CDS.VizieR/J/ApJ/707/L56</identifier><altIdentifier>doi:10.26093/cds/vizier.17079056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kovalev Y.Y.</name></creator><date role="Updated">2026-07-02T11:57:44Z</date><date role="Created">2012-02-02T14:40:06Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>gamma-ray-astronomy</subject><subject>radio-continuum-emission</subject><subject>astronomical-object-identification</subject><description>A list of 205 {gamma}-ray strong objects was reported recently as a result of a three-month integration with the Large Area Telescope on board the Fermi Gamma-Ray Space Telescope. We attempted identification of these objects, cross-correlating the {gamma}-ray positions with very long baseline interferometry (VLBI) positions of a large all-sky sample of extragalactic radio sources selected on the basis of their parsec-scale flux density. The original associations reported by the Fermi team are confirmed, and six new identifications are suggested. A Monte Carlo analysis shows that the fraction of chance associations in our analysis is less than 5%, and confirms that the vast majority of {gamma}-ray bright extragalactic sources are radio-loud blazars with strong parsec-scale jets. A correlation between the parsec-scale radio and {gamma}-ray flux is supported by our analysis of a complete VLBI flux-density-limited sample of extragalactic jets. The effectiveness of using a VLBI catalog to find associations between {gamma}-ray detections and compact extragalactic radio sources, especially near the Galactic plane, is demonstrated. It is suggested that VLBI catalogs should be used for future identification of Fermi/LAT objects.</description><source format="bibcode">2009ApJ...707L..56K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/707/L56</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/251">I/251 : VLBI International Celestial Reference Frame (ICRF) (Ma+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/405">J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/46">J/ApJS/183/46 : Fermi/LAT bright gamma-ray source list (0FGL) (Abdo+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/580">J/AJ/136/580 : Sixth VLBA calibrator survey: VCS6 (Petrov+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1236">J/AJ/133/1236 : Fifth VLBA calibrator survey: VCS5 (Kovalev+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1872">J/AJ/131/1872 : Fourth VLBA calibrator survey: VCS4 (Petrov+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/1163">J/AJ/129/1163 : Third VLBA calibrator survey: VCS3 (Petrov+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/3587">J/AJ/127/3587 : VLBI ICRF. 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